37 citations · 129 across the 7 of their papers we have counts for
7 papers
Active moons in our Solar System and beyond -- Io, Europa, Enceladus, Triton, and exomoons
Caroline Haslebacher, Emeline Bolmont, Marco Cilibrasi +19
The outgassing signatures of Io, Europa, Enceladus, Triton, and Io-like exomoons are the focus of this review chapter. The rocky volcanic world of Io is unique in our Solar System,…
Meridional Circulation driven by Planetary Spiral Wakes in Radiative and Magnetized Protoplanetary Discs
Marco Cilibrasi, Mario Flock, Judit Szulágyi
We study a Jupiter-mass planet formation for the first time in radiative magneto-hydrodynamics (MHD) simulations and compare it with pure hydrodynamical simulations, as well as to…
Did Uranus' regular moons form via a rocky giant impactor?
Jason Man Yin Woo, Christian Reinhardt, Marco Cilibrasi +3
The formation of Uranus' regular moons has been suggested to be linked to the origin of its enormous spin axial tilt (~98^o). A giant impact between proto-Uranus and a 2-3 M_Earth…
An N-body population synthesis framework for the formation of moons around Jupiter-like planets
Marco Cilibrasi, Judit Szulágyi, Simon L. Grimm +1
The moons of giant planets are believed to form in situ in Circumplanetary Discs (CPDs). Here we present an N-body population synthesis framework for satellite formation around a J…
Formation of satellites in circumplanetary discs generated by disc instability
C. Inderbitzi, J. Szulágyi, M. Cilibrasi +1
We investigated the formation and evolution of satellite systems in a cold, extended circumplanetary disc around a 10 gas giant which was formed by gravitational…
In Situ Formation of Icy Moons of Uranus and Neptune
J. Szulágyi, M. Cilibrasi, L. Mayer
Satellites of giant planets thought to form in gaseous circumplanetary disks (CPDs) during the late planet-formation phase, but it was unknown so far whether smaller mass planets,…
Satellites Form Fast & Late: a Population Synthesis for the Galilean Moons
M. Cilibrasi, J. Szulágyi, L. Mayer +3
The satellites of Jupiter are thought to form in a circumplanetary disc. Here we address their formation and orbital evolution with a population synthesis approach, by varying the…